Search Results - "Br\üggen, M"

Magnetic Field Amplification in Galaxy Clusters and Its Simulation by Donnert, J., Vazza, F., Brüggen, M., ZuHone, J.

“…We review the present theoretical and numerical understanding of magnetic field amplification in cosmic large-scale structure, on length scales of galaxy…”
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Analytical model for cluster radio relics by Brüggen, M, Vazza, F

“…ABSTRACT Radio relics are vast synchrotron sources that sit on the outskirts of merging galaxy clusters. In this work we model their formation using a…”
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Diffuse Radio Emission from Galaxy Clusters by van Weeren, R. J., de Gasperin, F., Akamatsu, H., Brüggen, M., Feretti, L., Kang, H., Stroe, A., Zandanel, F.

“…In a growing number of galaxy clusters diffuse extended radio sources have been found. These sources are not directly associated with individual cluster…”
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Do radio relics challenge diffusive shock acceleration? by Vazza, F., Brüggen, M.

“…Radio relics in galaxy clusters are thought to be associated with powerful shock waves that accelerate particles via diffusive shock acceleration (DSA). Among…”
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Resolved magnetic dynamo action in the simulated intracluster medium by Vazza, F., Brunetti, G., Brüggen, M., Bonafede, A.

“…Abstract Faraday rotation and synchrotron emission from extragalactic radio sources give evidence for the presence of magnetic fields extending over ∼ Mpc…”
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A radio ridge connecting two galaxy clusters in a filament of the cosmic web by Govoni, F, Orrù, E, Bonafede, A, Iacobelli, M, Paladino, R, Vazza, F, Murgia, M, Vacca, V, Giovannini, G, Feretti, L, Loi, F, Bernardi, G, Ferrari, C, Pizzo, R F, Gheller, C, Manti, S, Brüggen, M, Brunetti, G, Cassano, R, de Gasperin, F, Enßlin, T A, Hoeft, M, Horellou, C, Junklewitz, H, Röttgering, H J A, Scaife, A M M, Shimwell, T W, van Weeren, R J, Wise, M

“…Galaxy clusters are the most massive gravitationally bound structures in the Universe. They grow by accreting smaller structures in a merging process that…”
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On the amplification of magnetic fields in cosmic filaments and galaxy clusters by Vazza, F., Brüggen, M., Gheller, C., Wang, P.

“…The amplification of primordial magnetic fields via a small-scale turbulent dynamo during structure formation might be able to explain the observed magnetic…”
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Testing cosmic ray acceleration with radio relics: a high-resolution study using MHD and tracers by Wittor, D, Vazza, F, Brueggen, M

“…Weak shocks in the intracluster medium may accelerate cosmic-ray protons and cosmic-ray electrons differently depending on the angle between the upstream…”
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New constraints on the magnetization of the cosmic web using LOFAR Faraday rotation observations by O’Sullivan, S P, Brüggen, M, Vazza, F, Carretti, E, Locatelli, N T, Stuardi, C, Vacca, V, Vernstrom, T, Heald, G, Horellou, C, Shimwell, T W, Hardcastle, M J, Tasse, C, Röttgering, H

“…ABSTRACT Measuring the properties of extragalactic magnetic fields through the effect of Faraday rotation provides a means to understand the origin and…”
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Deep VLA Observations of the Cluster 1RXS J0603.3+4214 in the Frequency Range of 1-2 GHz by Rajpurohit, K., Hoeft, M., van Weeren, R. J., Rudnick, L., Röttgering, H. J. A., Forman, W. R., Brüggen, M., Croston, J. H., Andrade-Santos, F., Dawson, W. A., Intema, H. T., Kraft, R. P., Jones, C., Jee, M. James

“…We report L-band VLA observations of 1RXS J0603.3+4214, a cluster that hosts a bright radio relic, known as the Toothbrush, and an elongated giant radio halo…”
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Turbulent pressure support and hydrostatic mass bias in the intracluster medium by Angelinelli, M, Vazza, F, Giocoli, C, Ettori, S, Jones, T W, Brunetti, G, Brüggen, M, Eckert, D

“…ABSTRACT The degree of turbulent pressure support by residual gas motions in galaxy clusters is not well known. Mass modelling of combined X-ray and…”
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Analysis of anti‐tumour necrosis factor‐induced skin lesions reveals strong T helper 1 activation with some distinct immunological characteristics by Stoffel, E., Maier, H., Riedl, E., Brüggen, M.‐C., Reininger, B., Schaschinger, M., Bangert, C., Guenova, E., Stingl, G., Brunner, P.M.

“…Summary Background Psoriasiform and eczematous eruptions are the most common dermatological adverse reactions linked to anti‐tumour necrosis factor (TNF)‐α…”
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Constraining the efficiency of cosmic ray acceleration by cluster shocks by Vazza, F., Brüggen, M., Wittor, D., Gheller, C., Eckert, D., Stubbe, M.

“…We study the acceleration of cosmic rays by collisionless structure formation shocks with enzo grid simulations. Data from the Fermi satellite enable the use…”
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Properties of gas clumps and gas clumping factor in the intra-cluster medium by Vazza, F., Eckert, D., Simionescu, A., Brüggen, M., Ettori, S.

“…The spatial distribution of gas matter inside galaxy clusters is not completely smooth, but may host gas clumps associated with substructures. These overdense…”
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Shock–multicloud interactions in galactic outflows – II. Radiative fractal clouds and cold gas thermodynamics by Banda-Barragán, W E, Brüggen, M, Heesen, V, Scannapieco, E, Cottle, J, Federrath, C, Wagner, A Y

“…ABSTRACT Galactic winds are crucial to the cosmic cycle of matter, transporting material out of the dense regions of galaxies. Observations show the…”
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Turbulence and vorticity in Galaxy clusters generated by structure formation by Vazza, F, Jones, T W, Brueggen, M, Brunetti, G, Gheller, C, Porter, D, Ryu, D

“…Turbulence is a key ingredient for the evolution of the intracluster medium, whose properties can be predicted with high-resolution numerical simulations. We…”
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Morphology of radio relics – I. What causes the substructure of synchrotron emission? by Domínguez-Fernández, P, Brüggen, M, Vazza, F, Banda-Barragán, W E, Rajpurohit, K, Mignone, A, Mukherjee, D, Vaidya, B

“…ABSTRACT High-resolution radio observations of cluster radio relics often show complex spatial and spectral features. However, it is not clear what these…”
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The turbulent pressure support in galaxy clusters revisited by Vazza, F, Angelinelli, M, Jones, T W, Eckert, D, Brüggen, M, Brunetti, G, Gheller, C

“…ABSTRACT Due to their late formation in cosmic history, clusters of galaxies are not fully in hydrostatic equilibrium and the gravitational pull of their mass…”
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Measurements and simulation of Faraday rotation across the Coma radio relic by Bonafede, A., Vazza, F., Brüggen, M., Murgia, M., Govoni, F., Feretti, L., Giovannini, G., Ogrean, G.

“…The aim of this work is to probe the magnetic field properties in relics and infall regions of galaxy clusters using Faraday rotation measures. We present Very…”
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Simulations of ultra-high energy cosmic rays in the local Universe and the origin of cosmic magnetic fields by Hackstein, S, Vazza, F, Brüggen, M, Sorce, J G, Gottlöber, S

“…We simulate the propagation of cosmic rays at ultra-high energies, ≳10^18 eV, in models of extragalactic magnetic fields in constrained simulations of the…”
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